非局域磁捕获共振现象对回旋激射的影响

讨论磁镜场中弱相对论捕获电子的非局域磁捕获共振现象对回旋激射的影响。在高能电子分量与冷背景等离子体分量相比为一小量的近似下，用解析方法研究了回旋捕获共振所导致的沿磁力线传播的回旋激射，其结果与局域理论比较，发现非局域效应有很强的抑制作用。     

Detection of water masers in a sample of 84 IRAS sources

Using a newly installed system on the 25 m telescope of Urumqi Observatory, we searched for H20 maser emission towards 84 IRAS sources including young stellar objects （YSOs） and candidates for OFUIR stars. Water masers were detected in four star formation regions and one envelope of late type of stars for the first time. New water maser components were measured in two sources. In a maser source with no water maser emission detected six years ago, strong maser emission was found at different velocities, showing that there was a new explosion of water maser in this source.     

SiO脉泽源在银河系中的分布和空间运动

通过对日本野边山射电天文台45m望远镜探测到的453颗SiO脉泽源的相关数据进行分析和处理，研究了SiO脉泽源在银河系中的分布和运动学特征。     

被动型氢原子钟储存泡口原子分布计算及应用

为了获得被动型氢原子钟高、低能态氢原子经四极磁选态器偏转后在储存泡口的分布规律,建立了更加贴近实际情况的分布模型.利用统计学方法,一定温度下的氢原子出射速度采用麦克斯韦分布,出射角度近似采用均匀分布,并结合氢原子在四极磁选态系统中的运动规律,通过数值计算得到了距四极磁选态器出口一定距离处高、低能态氢原子的三维分布密度.应用该分布模型,计算得到收集高能态氢原子的泡口优化半径与聚焦距离之间的关系,为储存泡的加工和聚焦距离的设计提供了依据,可以使得高能态原子被最大程度聚集,低能态原子被偏离,从而提高谐振腔内跃迁信号的功率.     

On theories of solar type III radio bursts

In solar radiophysics,many theories for type Ⅲ bursts have been proposed during the past 60 years.Almost all these theories are based on the plasma hypothesis,which assumes that(i)the radiation is mainly generated by Langmuir waves via nonlinear processes and(ii)the radiation has frequencies close to the local plasma frequency and/or its second harmonic in the source region. We feel strongly that it is time to advocate an alternative approach without recourse to the plasma hypothesis.This brief discussion explains why.     

CARM放大器回旋动力学理论及其与实验的比较

对圆柱腔回旋自动谐振脉塞(CARM)回旋动力学理论与美国麻省理工学院的实验进行了比较研究,理论结果与实验符合。研究了磁场及电子横向速度与纵向速度比对输出功率和增益的影响,发现通过优化参数,原实验的输出功率有可能从10MW提高到14MW。     

活动星系核水脉泽源的谱能量分布

收集目前发表的与活动星系核相关的所有水脉泽源,以及它们各个波段(从射电到X射线)的观测资料.在66个这类星系中,有40个源的观测资料较全,得到的谱能量分布图较好,便于进一步分析.它们的谱能量分布形态相似,最强辐射位于远红外波段(峰值出现在～ 60 μm处).对它们的谱能量分布图进行拟合积分,估计得到它们的热光度.热光度范围从1042到1046 ergs·s-1,且大多数(26/40)为～1044ergs·s-1,平均值为1044.4±0 1 ergs·s-1.对这40个源的子样本,进一步分析其脉泽辐射强度与脉泽寄主星系热光度间的可能的相关.结果显示,虽然弥散比较大,但脉泽辐射随热光度增加趋向于增强.对影响这一相关性的可能因素做进一步讨论.     

河外水脉泽寄主星系的射电谱指数(英文)

详细调研并收集了所有河外水脉泽寄主星系的射电观测资料(84个源).在6 cm和20 cm两个波段,"千脉泽"(其光度小于10个太阳光度)源的射电流量都大于"兆脉泽"源(其光度大于10个太阳光度).由收集的这两个波段的观测数据,首次导出了水脉泽星系的射电谱指数,α=0.87±0.11.比较水脉泽星系和没有检测到水脉泽的星系的谱指数,没有发现明显的差异.进一步分析水脉泽各向同性辐射光度与脉泽寄主星系射电强度,发现它们之间存在一个强相关,这与水脉泽辐射可能是对背景射电连续谱的放大的理论结果相吻合.     

Research on frequency-temperature compensated sapphire-SrTiO3 loaded cavity for hydrogen maser

To obtain frequency-temperature compensation in a sapphire loaded cavity for hydrogen maser, a dielectric named SrTiO3 is employed whose temperature coefficient of permittivity is opposite to that of sapphire. Based on theoretical analysis and computer simulation, a TE011 mode of a sapphire loaded cavity associated with two small rings of SrTiO3 with different thickness is solved, and the useful parameters that influence the temperature coefficient of cavity are calculated. Finally an experiment is brought forward and its results are very close to the computing results. When the thickness of SiTiO3 dielectric is 7 mm and the diameter is 17 mm in configuration b, the temperature coefficient of cavity is decreased from −58.8 kHz/K to −8.2 kHz/K and the quality factor is 40248.